Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
A confirmed deficit of hot and cold dust emission in the most luminous Little Red Dots
As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 22 inbound Pith citation observations for arXiv:2503.02059.
A citation records a reference. It does not transfer a finding from one paper to another.
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One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-10T06:31:04.303077+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-08T16:36:20.434406Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-07-10T12:15:01.137692Z
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0 of 0 outbound references displayed
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Outbound references
No outbound reference observations are available for this paper version.
Pith citing papers
Observation ce3df3d4-e266-4f91-bf4d-83f5b63b15ef · inbound
Investigating photometric and spectroscopic variability in the multiply-imaged Little Red Dot A2744-QSO1 cites this paper.
Investigating photometric and spectroscopic variability in the multiply-imaged Little Red Dot A2744-QSO1 A confirmed deficit of hot and cold dust emission in the most luminous Little Red Dots
Reference 84
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T11:37:36.535246Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation c43ffdd5-73bc-4150-bf36-687199f65fc2 · inbound
A "Black Hole Star" Reveals the Remarkable Gas-Enshrouded Hearts of the Little Red Dots cites this paper.
A "Black Hole Star" Reveals the Remarkable Gas-Enshrouded Hearts of the Little Red Dots A confirmed deficit of hot and cold dust emission in the most luminous Little Red Dots
Reference 59
- Resolution
- verified exact
- arxiv_id, observed 2026-05-16T08:53:14.812889Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation 55f8bccd-98e4-42ca-a995-5e22ce26ee03 · inbound
An upper limit of 10$^6$ M$_\odot$ in dust from ALMA observations in 60 Little Red Dots cites this paper.
An upper limit of 10$^6$ M$_\odot$ in dust from ALMA observations in 60 Little Red Dots A confirmed deficit of hot and cold dust emission in the most luminous Little Red Dots
Reference 29
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T14:31:04.155899Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 19cb913f-bce2-4ce4-b2bb-21427426c4ff · inbound
Realistic Multi-temperature Dust: How Well Can We Constrain the Dust Properties of High-redshift Galaxies? cites this paper.
Realistic Multi-temperature Dust: How Well Can We Constrain the Dust Properties of High-redshift Galaxies? A confirmed deficit of hot and cold dust emission in the most luminous Little Red Dots
Reference 132
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T14:06:33.979919Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 7e67b7ca-4cb6-43fa-bc40-79131ec2c3a2 · inbound
Beneath the Surface: >85% of z>5.9 QSOs in Massive Host Galaxies are UV-Faint cites this paper.
Beneath the Surface: >85% of z>5.9 QSOs in Massive Host Galaxies are UV-Faint A confirmed deficit of hot and cold dust emission in the most luminous Little Red Dots
Reference 84
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T21:45:23.464534Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 556274fc-aec5-4f76-808e-e22e49cb34a0 · inbound
Little Red reionization factories cites this paper.
Little Red reionization factories A confirmed deficit of hot and cold dust emission in the most luminous Little Red Dots
Reference 24
- Resolution
- unresolved
- no resolver link, observed 2026-08-05T19:03:20.136689Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 43b12d88-4eb3-400a-bb6b-de4ea69c1bf4 · inbound
Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). XXIV. 54 New Quasars and Candidate Obscured Quasars at $5.71 \le z \le 7.02$ cites this paper.
Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). XXIV. 54 New Quasars and Candidate Obscured Quasars at $5.71 \le z \le 7.02$ A confirmed deficit of hot and cold dust emission in the most luminous Little Red Dots
Reference 141
- Resolution
- unresolved
- no resolver link, observed 2026-08-05T14:33:59.024627Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation fa391c41-c6cb-43ca-8143-9dd281978cf5 · inbound
Do Little Red Dots Vary? cites this paper.
Do Little Red Dots Vary? A confirmed deficit of hot and cold dust emission in the most luminous Little Red Dots
Reference 66
- Resolution
- unresolved
- no resolver link, observed 2026-08-05T10:54:53.307276Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 59b653b3-e742-4b90-ac93-7e3cff5cbd37 · inbound
What you see is what you get: empirically measured bolometric luminosities of Little Red Dots cites this paper.
What you see is what you get: empirically measured bolometric luminosities of Little Red Dots A confirmed deficit of hot and cold dust emission in the most luminous Little Red Dots
Reference 69
- Resolution
- unresolved
- no resolver link, observed 2026-08-05T05:29:30.183520Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation f3849e47-d355-44da-97ab-c545d4775c12 · inbound
Spectral Uniformity of Little Red Dots: A Natural Outcome of Coevolving Seed Black Holes and Nascent Starbursts cites this paper.
Spectral Uniformity of Little Red Dots: A Natural Outcome of Coevolving Seed Black Holes and Nascent Starbursts A confirmed deficit of hot and cold dust emission in the most luminous Little Red Dots
Reference 129
- Resolution
- verified exact
- arxiv_id, observed 2026-05-18T14:41:29.550015Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation ed8509c8-188d-49d2-bec3-2b607755b291 · inbound
Evidence of violation of Case B recombination in Little Red Dots cites this paper.
Evidence of violation of Case B recombination in Little Red Dots A confirmed deficit of hot and cold dust emission in the most luminous Little Red Dots
Reference 52
- Resolution
- unresolved
- no resolver link, observed 2026-08-04T11:17:07.820165Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 99cec957-8923-4628-9734-26644ed3880b · inbound
VENUS: When Red meets Blue -- A multiply imaged Little Red Dot with an apparent blue companion behind the galaxy cluster Abell 383 cites this paper.
VENUS: When Red meets Blue -- A multiply imaged Little Red Dot with an apparent blue companion behind the galaxy cluster Abell 383 A confirmed deficit of hot and cold dust emission in the most luminous Little Red Dots
Reference 61
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T19:07:29.233429Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 52ab4a9b-e90d-4382-9891-c5cf55d5db88 · inbound
Little Red Dots as Hidden Neutrino Sources cites this paper.
Little Red Dots as Hidden Neutrino Sources A confirmed deficit of hot and cold dust emission in the most luminous Little Red Dots
Reference 98
- Resolution
- verified exact
- arxiv_id, observed 2026-05-16T13:42:56.303525Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation 0816cc99-9b60-425b-8614-3dbca246cfc6 · inbound
Quenching of X-ray emission in little red dots by both Compton-thick gas and high accretion rates cites this paper.
Quenching of X-ray emission in little red dots by both Compton-thick gas and high accretion rates A confirmed deficit of hot and cold dust emission in the most luminous Little Red Dots
Reference 57
- Resolution
- metadata mismatch
- arxiv_id, observed 2026-05-19T16:22:39.218139Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation 594f0b09-0329-457d-8a3b-d3bc92cbaddb · inbound
(LRDs)$^2$: The Low-ReDshift Little Red Dots Survey. II. DESI DR1 Sample cites this paper.
(LRDs)$^2$: The Low-ReDshift Little Red Dots Survey. II. DESI DR1 Sample A confirmed deficit of hot and cold dust emission in the most luminous Little Red Dots
Reference 122
- Resolution
- verified exact
- arxiv_id, observed 2026-05-22T09:46:21.943488Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation d2e54572-96b1-4b85-a383-fe88420103aa · inbound
Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution cites this paper.
Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution A confirmed deficit of hot and cold dust emission in the most luminous Little Red Dots
Reference 20
- Resolution
- unresolved
- no resolver link, observed 2026-08-02T12:34:26.762937Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation d6eddd68-9b80-440c-8729-ef77059dffcc · inbound
Dust in the Average Galaxy: Attenuation, Emission, and Opacity from 0<z<7 cites this paper.
Dust in the Average Galaxy: Attenuation, Emission, and Opacity from 0<z<7 A confirmed deficit of hot and cold dust emission in the most luminous Little Red Dots
Reference 167
- Resolution
- verified exact
- arxiv_id, observed 2026-06-27T02:30:23.084305Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation df953e6f-c451-4275-8823-e132ae8a2351 · inbound
The metallicities of little red dot host galaxies: LRDs are metal poor, but not pristine cites this paper.
The metallicities of little red dot host galaxies: LRDs are metal poor, but not pristine A confirmed deficit of hot and cold dust emission in the most luminous Little Red Dots
Reference 197
- Resolution
- metadata mismatch
- arxiv_id, observed 2026-07-01T05:05:24.239818Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation f3d3927b-2738-4c49-9d82-b02378e402b4 · inbound
Little Red Dots at z~2 in EIGER reveal a gentle decline with respect to their peak number density at z~5 cites this paper.
Little Red Dots at z~2 in EIGER reveal a gentle decline with respect to their peak number density at z~5 A confirmed deficit of hot and cold dust emission in the most luminous Little Red Dots
Reference 61
- Resolution
- metadata mismatch
- arxiv_id, observed 2026-07-02T18:27:16.552664Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation 52a9e234-d273-42d7-a74b-609409a78f76 · inbound
ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs cites this paper.
ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs A confirmed deficit of hot and cold dust emission in the most luminous Little Red Dots
Reference 56
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T00:25:30.130342Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 745e0e66-6a4a-4d90-b8a5-0b0bd8056fc3 · inbound
Misaligned or chaotic? A strong break of axial symmetry in the local LRD J1025 revealed with VLT/FORS2 spectropolarimetry cites this paper.
Misaligned or chaotic? A strong break of axial symmetry in the local LRD J1025 revealed with VLT/FORS2 spectropolarimetry A confirmed deficit of hot and cold dust emission in the most luminous Little Red Dots
Reference 145
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T00:41:30.865906Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation e41f3e4e-9ce1-4b56-af3c-ada6a20117f7 · inbound
Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ cites this paper.
Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ A confirmed deficit of hot and cold dust emission in the most luminous Little Red Dots
Reference 63
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T16:36:20.434406Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.